Kepler-1067 c
Astrophysical Synthesis & Habitability Characterization
Kepler-1067 c is a confirmed super-earth exoplanet orbiting the star Kepler-1067, located approximately 2177.7 light-years (667.69 parsecs) from the Solar System. First announced in 2021 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0294% across the stellar disk), this world measures 1.747 Earth radii and has a measured mass of 3.7 Earth masses. Combining its mass and radius yields a mean bulk density of 3.83 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.21 g⊕ (11.87 m/s²), and an escape velocity of 16.3 km/s.
In its orbital architecture around Kepler-1067, Kepler-1067 c completes one full revolution every 5.426 Earth days at a semi-major axis of 0.06069 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 121.7 km/s (compared to Earth's 29.8 km/s). The orbit is modeled as circular (e = 0.00), maintaining a constant stellar distance throughout its year.
⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 973 K (+700°C / +1292°F) and receiving 190.80 S⊕ (~259,679 W/m²), Kepler-1067 c orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-1067 is classified as a stellar host with an effective photospheric temperature of 5,594 K, a radius of 0.934 R☉, a mass of 0.981 M☉, an estimated bolometric luminosity of 0.766 L☉. Stellar evolution modeling indicates an estimated stellar age of 0.81 Gyr and a metallicity of [Fe/H] = 0.16 dex (metal-rich relative to the Sun). From Earth, Kepler-1067 shines at apparent V-band magnitude 14.395 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The Kepler-1067 system is a multi-planet architecture hosting 2 confirmed worlds, with Kepler-1067 c sharing its stellar neighborhood alongside Kepler-1067 b.
Methodology: Computed using the Schulze-Makuch et al. (2011) weighted metric comparing physical interior (radius, estimated density) and surface thermal regime (escape velocity, equilibrium temperature).
Discovery Facility: Kepler · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).
☀️ Host Star Telemetry
| Host Star Name | Kepler-1067 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,594 K |
| Stellar Radius | 0.9340 R☉ |
| Stellar Mass | 0.9810 M☉ |
| Bolometric Luminosity | 0.766 L☉ |
| Metallicity [Fe/H] | 0.160 dex |
| Stellar Age | 0.810 Gyr |
| Apparent Magnitude | V: 14.395 · G: 14.273 |
| System Architecture | 1 Star, 2 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.060690 AU |
| Orbital Period | 5.426 days |
| Mean Orbital Velocity | 121.7 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.6500° |
| Mean Bulk Density | 3.83 g/cm³ (16.3 km/s vesc) |
| Insolation Flux | 190.8000 S⊕ (~259,679 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 2177.700 LY (667.693 pc) |